Separation of noisy astrophysical images by blind time-frequency source separation methods;Gürültülü astroflziksel görüntü karişimlannin kör zaman-siklik kaynak ayriştirma yöntemleri ile ayriştirilmasi

2007 IEEE 15th Signal Processing and Communications Applications, SIU

Volumn , Issue , 2007, Pages

  Özgen, Mehmet Tankut ^a   Herranz, Diego ^b   Kuruoglu, Ercan Engin ^c  

^a ANADOLU UNIVERSITY   (Turkey)

^b INSTITUTO DE FÍSICA DE CANTABRIA CSIC UC   (Spain)

^c ISTI CNR   (Italy)

Author keywords

[No Author keywords available]

Indexed keywords

ASTROPHYSICS; COSMOLOGY; FOOD ADDITIVES; ISOMERS; MIXTURES; MODELS; PARTICLE ACCELERATORS; SEPARATION; SIGNAL ANALYSIS; SIGNAL PROCESSING; SYNCHROTRONS;

BLIND TIME; COSMIC MICROWAVE BACKGROUND RADIATION; FASTICA ALGORITHMS; GAUSSIAN NOISE; NON-STATIONARY; PHYSICAL MODELLING; POWER LEVELING;

BLIND SOURCE SEPARATION;

EID: 50249175069     PISSN: None     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1109/SIU.2007.4298795     Document Type: Conference Paper

References (7)

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7. A. Yeredor, "Non-orthogonal joint diagonalization in the least-squares sense with application in blind source separation," IEEE Trans. Signal Process., vol. 50, no. 7, pp. 1545-1553, 2002.